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Cosmic web analysis and information theory some recent results Florent Leclercq Institute of Cosmology and Gravitation, University of Portsmouth January 5 th , 2016 In collaboration with: Jens Jasche (ExC Universe, Garching), Guilhem Lavaux (IAP), Will Percival (ICG), Benjamin Wandelt (IAP/U. Illinois) 1
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Page 1: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

Cosmic web analysis and information theorysome recent results

Florent LeclercqInstitute of Cosmology and Gravitation, University of Portsmouth

January 5th, 2016

In collaboration with:Jens Jasche (ExC Universe, Garching), Guilhem Lavaux (IAP),

Will Percival (ICG), Benjamin Wandelt (IAP/U. Illinois)

1

Page 2: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

Uncertainty quantification

2

Can we uncertainty

quantification to ?

Uncertainty quantification is crucial!

Yes, and this is what yields a connection

with !

Page 3: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

Cosmic web classification procedures

3

• The :

uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational potential:

Hahn et al. 2007, arXiv:astro-ph/0610280

void, sheet, filament, cluster?

Page 4: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

4

Final conditions

FL, Jasche & Wandelt 2015, arXiv:1502.02690

T-web structures inferred by BORG

Page 5: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

5

Initial conditions

FL, Jasche & Wandelt 2015, arXiv:1502.02690

T-web structures inferred by BORG

Page 6: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

What is the information content of these maps?

6

in shannons (Sh)

Initial conditionsFinal conditions

FL, Jasche & Wandelt 2015, arXiv:1502.02690

Shannon entropy

Page 7: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

How much did the data surprise us?

7

Initial conditionsFinal conditions

in Sh

FL, Jasche & Wandelt 2015, arXiv:1502.02690

information gain a.k.a. relative entropy or Kullback-Leibler divergence posterior/prior

Page 8: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

A decision rule for structure classification

• Space of “input features”:

• Space of “actions”:

• A problem of :one should take the action that maximizes the utility

• How to write down the gain functions?

8FL, Jasche & Wandelt 2015, arXiv:1503.00730

Page 9: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

• One proposal:

• Without data, the expected utility is

• With , it’s a fair game always play

“ ” of the LSS

• Values represent an aversion for risk

increasingly “ ” of the LSS

Gambling with the Universe

9

“Winning”

“Loosing”

“Not playing”

“Playing the game”

“Not playing the game”

FL, Jasche & Wandelt 2015, arXiv:1503.00730

voidssheetsfilamentsclusters

1.74

7.08

3.83

41.67(T-web, final conditions)

Page 10: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

Playing the game…

10

Final conditions

voids

sheets

filaments

clusters

undecided

Initial conditions

FL, Jasche & Wandelt 2015, arXiv:1503.00730

Page 11: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

Cosmic web classification procedures

12

• The :

uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational potential:

• :

uses the sign of : eigenvalues of the shear of the Lagrangian displacement field:

• :

uses the dark matter “phase-space sheet” (number of orthogonal axes along which there is shell-crossing)

Hahn et al. 2007, arXiv:astro-ph/0610280

Lavaux & Wandelt 2010, arXiv:0906.4101

Falck, Neyrinck & Szalay 2012, arXiv:1201.2353

Lagrangianclassifiers

void, sheet, filament, cluster?

now usable in real data!

Page 12: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

13

Comparing classifiersFi

lam

ents

Void

s

FL, Jasche & Wandelt 2015, arXiv:1502.02690

FL, Jasche, Lavaux & Wandelt 2016, arXiv:1601.00093

Page 13: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

How similar are different classifications?

14FL, Lavaux, Jasche & Wandelt, in prep.

Jensen-Shannon divergence

(more about the Jensen-Shannon divergence later)

Page 14: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

Which is the best classifier?

• Can we extend the decision problem to the space of classifiers?

• As before, the idea is to maximize a utility function

• An important notion: the between two random variables

• Property:

15

Mutual information is the expectation of the Kullback-Leibler divergence of the conditional from the unconditional distribution.

FL, Lavaux, Jasche & Wandelt, in prep.

Page 15: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

1. Utility for parameter inference:cosmic web analysis• In analogy with the formalism of

: maximize the for cosmic web maps

16FL, Lavaux, Jasche & Wandelt, in prep.

classification data

Page 16: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

2. Utility for model selection:dark energy equation of state

• For example, consider three dark energy models with

• The between posterior predictive distributions can be used as an approximate

• In analogy:

17

model classifier mixture distribution

Vanlier et al. 2014, BMC Syst Biol 8, 20 (2014)

FL, Lavaux, Jasche & Wandelt, in prep.

Page 17: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

3. Utility for prediction of new data:galaxy colors

• Maximize the for some new quantity

18

predicted data classification

FL, Lavaux, Jasche & Wandelt, in prep.

Page 18: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

3. Utility for prediction of new data:galaxy colors

• How to compute the information gain?

19

parent entropy:

child2 entropy:

child1 entropy:

weighted average entropy of children:

information gain for this split:

Page 19: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

3. Utility for prediction of new data:galaxy colors

• A problem!

• 3 = classifications (T-web, DIVA, ORIGAMI) with

• 4 (void, sheet, filament, cluster)

• 2 (red, blue)

20

X Y Z C

3 2 3 I

3 1 3 I

2 2 0 II

3 1 0 II

no gain: worst best!

X=3

Y=0

Y=1

Y=2

Y=3

Z=0

Z=1

Z=2

Z=3

X=0

X=1

X=2

FL, Lavaux, Jasche & Wandelt, in prep.

Page 20: Cosmic web analysis and information theory · Cosmic web classification procedures 12 •The : uses the sign of : eigenvalues of the tidal field tensor, Hessian of the gravitational

Conclusions

• Thanks to , the can be described using various classifiers

• Probabilistic analysis of the cosmic web yields a data-supported

offers a framework to classify structures in the presence of uncertainty

• It is now possible to !

• The decision problem can be extended to the , with utility functions depending on the desired use

(Some numerical results for classifier utilities in the upcoming paper)

21FL, Lavaux, Jasche & Wandelt, in prep.

FL, Jasche, Lavaux & Wandelt 2016, arXiv:1601.00093

FL, Jasche & Wandelt 2015, arXiv:1503.00730


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